probability densities of the effective neutrino masses mβ and mββ

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2017
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Abstract
We compute the probability densities of the effective neutrino masses mβ and mββ using the Kernel Density Estimate (KDE) approach applied to a distribution of points in the (mmin,mββ) and (mβ,mββ) planes, obtained using the available Probability Distribution Functions (PDFs) of the neutrino mixing angles and mass differences, with the additional constraints coming from cosmological data on the sum of the neutrino masses. We show that the reconstructed probability densities strongly depend on the assumed set of cosmological data: for ∑jmj≤0.68 eV at 95%CL a sensitive portion of the allowed values are already excluded by null results of experiments searching for mββ and mβ, whereas in the case ∑jmj≤0.23 eV at 95%CL the bulk of the probability densities are below the current bounds.
Reference Key
iura2017nuclearprobability Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;Andrea Di Iura;Davide Meloni
Journal biology and fertility of soils
Year 2017
DOI
10.1016/j.nuclphysb.2017.06.015
URL
http://www.sciencedirect.com/science/article/pii/S0550321317302109
Keywords
radioactivity atomic energy nuclear and particle physics

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